activity
20082026
most citedThe Kuiper Belt Luminosity Function from m(R)=21 to 26

106 citations · 358 across the 10 of their papers we have counts for

collaborators

8 papers

astro-ph.EP2026

Linear Continuum Modelling to Explain The Majority of Bulk Features of Kuiper Belt Object Spectra

Wesley C. Fraser, Laura E. Buchanan, Ian Wong +2

The first analyses of the James Webb Space Telescope spectra of trans-Neptunian Objects (TNOs) revealed three discrete types of surfaces. This seems to contradict ground-based spec…

cs.CV2025

Moving object detection from multi-depth images with an attention-enhanced CNN

Masato Shibukawa, Fumi Yoshida, Toshifumi Yanagisawa +12

One of the greatest challenges for detecting moving objects in the solar system from wide-field survey data is determining whether a signal indicates a true object or is due to som…

astro-ph.EP2025★ 3 cited

JWST Spectroscopy of a Blue Binary Cold Classical Kuiper Belt Object

Ian Wong, Bryan J. Holler, Wesley C. Fraser +1

We present observations of two binary systems within the cold classical region of the Kuiper belt2001 XR254 and 2016 BP81obtained with the JWST Near-Infrared Spectrograph. Th…

astro-ph.EP2024

Detecting Moving Objects With Machine Learning

Wesley C. Fraser

The scientific study of the Solar System's minor bodies ultimately starts with a search for those bodies. This chapter presents a review of the use of machine learning techniques t…

astro-ph.EP2011★ 49 cited

The surface composition of large Kuiper belt object 2007 OR10

M. E. Brown, A. J. Burgasser, W. C. Fraser

We present photometry and spectra of the large Kuiper belt object 2007 OR10. The data show significant near-infrared absorption features due to water ice. While most objects in the…

astro-ph.EP2009★ 32 cited

NICMOS Photometry of the Unusual Dwarf Planet Haumea and its Satellites

W. C. Fraser, M. E. Brown

We present here HST NICMOS F110W and F160W observations of Haumea, and its two satellites Hi'iaka and Namaka. From the measured (F110W-F160W) colours of -1.209 +/-0.004, -1.48 +/-…